Determination of Object Thickness in Electron Microscopy
dc.contributor.author | Marton, L. | en_US |
dc.contributor.author | Schiff, L. I. | en_US |
dc.date.accessioned | 2010-05-06T22:55:07Z | |
dc.date.available | 2010-05-06T22:55:07Z | |
dc.date.issued | 1941-10 | en_US |
dc.identifier.citation | Marton, L.; Schiff, L. I. (1941). "Determination of Object Thickness in Electron Microscopy." Journal of Applied Physics 12(10): 759-765. <http://hdl.handle.net/2027.42/70918> | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/70918 | |
dc.description.abstract | It is proposed that the thicknesses of electron microscope objects be determined by measuring the diminution in intensity of the electron beam caused by the object. Since this method would only be applied to specimens so thin that multiple scattering can be neglected, one need know only the total cross section for single scattering of electrons outside the aperture angle of the electron microscope objective. These cross sections are calculated for fast electrons (energies greater than 10,000 ev) by means of the Born approximation for several cases of practical interest, and the results are applied to some experimental observations. | en_US |
dc.format.extent | 3102 bytes | |
dc.format.extent | 1079579 bytes | |
dc.format.mimetype | text/plain | |
dc.format.mimetype | application/pdf | |
dc.publisher | The American Institute of Physics | en_US |
dc.rights | © The American Institute of Physics | en_US |
dc.title | Determination of Object Thickness in Electron Microscopy | en_US |
dc.type | Article | en_US |
dc.subject.hlbsecondlevel | Physics | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | The Harrison M. Randall Laboratory of Physics, University of Michigan, Ann Arbor, Michigan | en_US |
dc.contributor.affiliationother | Randal Morgan Laboratory of Physics, University of Pennsylvania, Philadelphia, Pennsylvania | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/70918/2/JAPIAU-12-10-759-1.pdf | |
dc.identifier.doi | 10.1063/1.1712863 | en_US |
dc.identifier.source | Journal of Applied Physics | en_US |
dc.identifier.citedreference | See T. H. Osgood, J. App. Phys. 12, 96 (1941). | en_US |
dc.identifier.citedreference | This micrograph was taken by keeping the object stationary and changing the angle of incidence of the condenser beam, instead of the usual method of tilting the specimen. This could be done because of the relatively large apertures of the electron microscope used for taking these pictures (see also L. Marton, Phys. Rev. 58, 57 (1940)) and because the image quality is primarily defined by the solid angle of the incident (condenser) beam and not by the actual size of the objective aperture (due to the predominance of large angles in the scattered beam). (See also V. Borries and Ruska, Zeits. f. Tech. Physik 19, 404 (1938).) For stereophotogrammetric measurements see W. Eitel and E. Gotthardt, Naturwiss. 28, 367 (1940); smallest measured thickness 200A, accuracy ±50A.±50A. | en_US |
dc.identifier.citedreference | In contrast to a former paper where an estimation of “depth resolving power” was given by considering multiple scattering alone [L. Marton, Physica 9, 959 (1936)]. | en_US |
dc.identifier.citedreference | F. Seitz, Modern Theory of Solids (McGraw‐Hill, 1940), p. 72. | en_US |
dc.identifier.citedreference | N. F. Mott and H. S. W. Massey, Theory of Atomic Collisions (Oxford, 1933), p. 88. | en_US |
dc.identifier.citedreference | Reference 5, p. 124. | en_US |
dc.identifier.citedreference | Reference 5, Chapter XI, especially Eqs. (39), (38), (13), (7). The relativity modifications can be established by the method of impact parameters: E. J. Williams, Proc. Roy. Soc. A139, 163 (1933). | en_US |
dc.identifier.citedreference | J. C. Slater, Phys. Rev. 36, 57 (1930). | en_US |
dc.identifier.citedreference | G. W. Brindley, Phil. Mag. 11, 786 (1931); F. E. Hoare, Proc. Roy. Soc. A147, 88 (1934). | en_US |
dc.identifier.citedreference | J. B. H. Kuper, Phys. Rev. 53, 993 (1938). | en_US |
dc.identifier.citedreference | J. B. H. Kuper and E. Teller, Phys. Rev. 58, 602 (1940). | en_US |
dc.identifier.citedreference | See also reference 5, p. 270. | en_US |
dc.identifier.citedreference | E. J. Williams, Proc. Roy. Soc. A169, 531 (1939), | en_US |
dc.identifier.citedreference | S. Goudsmit and J. L. Saunderson, Phys. Rev. 58, 36 (1940). | en_US |
dc.identifier.citedreference | See, for instance, E. Perucca, Nuovo Cimento 15, 365 (1938); J. Strong and B. Dibble, J. Opt Soc. Am. 30, 431 (1940). | en_US |
dc.identifier.citedreference | L. Marton, J. W. McBain and R. D. Vold, J. Am. Chem. Soc. 63, 1990 (1941). | en_US |
dc.identifier.citedreference | Prepared by Dr. E. G. Ramberg. | en_US |
dc.owningcollname | Physics, Department of |
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